SDO HMI 2014-09-29 11:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.22 | 0.00 | 7.32 | -16.82 | 199.29 | -5.79 | 166.75 | 0.4291 | -282.8 | -205.6 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.50 | 0.00 | 0.83 | -18.36 | 214.39 | 9.30 | 199.91 | 0.4523 | 723.0 | 566.1 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -15.16 | 208.31 | 3.23 | 188.28 | 0.3790 | 799.0 | 524.8 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -16.05 | 203.39 | -1.70 | 175.80 | 0.3908 | -594.0 | -454.9 | |
| 0.00 | 1.68 | 0.00 | 0.89 | -14.63 | 202.16 | -2.93 | 172.29 | 0.3699 | -820.0 | -484.4 | |
| 0.00 | 1.85 | 0.00 | 1.00 | -16.65 | 201.81 | -3.27 | 172.16 | 0.4029 | -680.0 | -581.0 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -17.41 | 196.13 | -8.96 | 160.01 | 0.4364 | -550.0 | -550.6 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -17.28 | 196.01 | -9.08 | 159.65 | 0.4352 | -703.0 | -516.6 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -26.54 | 192.57 | -12.52 | 160.48 | 0.5825 | -704.0 | -567.7 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -6.77 | 193.83 | -11.26 | 140.13 | 0.3038 | 871.0 | 573.9 | |
| 0.00 | 1.41 | 0.00 | 0.74 | -6.98 | 192.93 | -12.16 | 138.37 | 0.3162 | -851.0 | -699.8 | |
| 0.00 | 1.06 | 0.00 | 0.72 | -31.48 | 183.36 | -21.73 | 152.71 | 0.6911 | -602.0 | -483.8 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |